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INTERNATIONAL JOURNAL OF NOVEL RESEARCH AND DEVELOPMENT International Peer Reviewed & Refereed Journals, Open Access Journal ISSN Approved Journal No: 2456-4184 | Impact factor: 8.76 | ESTD Year: 2016 Scholarly open access journals, Peer-reviewed, and Refereed Journals, Impact factor 8.76 (Calculate by google scholar and Semantic Scholar | AI-Powered Research Tool) , Multidisciplinary, Monthly, Indexing in all major database & Metadata, Citation Generator, Digital Object Identifier(DOI) |
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| Paper Title: | Spectroscopy of Cosmic Waves |
| Authors Name: | DEEYA SHALYA , DR.SURBHI MALIK |
| Download E-Certificate: | Download |
| Author Reg. ID: |
IJNRD_196089
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| Published Paper Id: | IJNRD2305531 |
| Published In: | Volume 8 Issue 5, May-2023 |
| DOI: | |
| Abstract: | When the universe began to form 13.8 billion years ago, the big bang triggered an enormous number of mutations. 40,000 years after the Big Bang, cosmologists discovered the cosmic microwave background, also known as the CMB. Once thought to be merely some heat radiation left over from the Big Bang, or the moment the universe originated, the cosmic microwave background (or CMB) was discovered. The universe is filled with a very faint glow of light, or radiation, known as Cosmic Microwave Background radiation, or CMB radiation for short. The CMB radiation falls on Earth from all directions with a remarkably uniform intensity. The maximal energy of cosmic rays accelerated in supernova remnants is limited and is determined by the size and strength of the acceleration region's magnetic field. The origin of these ultra-high energies is a major outstanding subject in astronomy because cosmic rays have been recorded at energies that are substantially greater than those produced by supernova remnants. They might originate from quasars, gamma-ray bursts, or active galactic nuclei that are outside of the galaxy. A mathematical procedure known as "blackbody radiation inversion" uses the determined power radiation spectrum to estimate the temperature probability distribution. To determine the temperature distribution of the producing medium, this inversion approach is used to invert the blackbody radiation field corresponding to the cosmic microwave background, which is the hot big bang's residual radiation. The key characteristics of this distribution are examined, and the study of this distribution suggests that the cosmic microwave background spectrum contains distortion. |
| Keywords: | Cosmic Microwave Background, Blackbody Radiation Inversion. |
| Cite Article: | "Spectroscopy of Cosmic Waves", International Journal of Novel Research and Development (www.ijnrd.org), ISSN:2456-4184, Vol.8, Issue 5, page no.f139-f145, May-2023, Available :http://www.ijnrd.org/papers/IJNRD2305531.pdf |
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2456-4184 | IMPACT FACTOR: 8.76 Calculated By Google Scholar| ESTD YEAR: 2016 An International Scholarly Open Access Journal, Peer-Reviewed, Refereed Journal Impact Factor 8.76 Calculate by Google Scholar and Semantic Scholar | AI-Powered Research Tool, Multidisciplinary, Monthly, Multilanguage Journal Indexing in All Major Database & Metadata, Citation Generator |
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Published Paper ID:IJNRD2305531 Registration ID: 196089 Published In: Volume 8 Issue 5, May-2023 DOI (Digital Object Identifier): Page No: f139-f145 Country: NOIDA (Gautam Budh Nagar), Uttar Pradesh, India Research Area: Physics Publisher : IJ Publication Published Paper URL : https://www.ijnrd.org/viewpaperforall?paper=IJNRD2305531 Published Paper PDF: https://www.ijnrd.org/papers/IJNRD2305531 |
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ISSN: 2456-4184
Impact Factor: 8.76 and ISSN APPROVED
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